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CMB-S4 Science Book, First Edition

Authors :
Nicholas Battaglia
Daniel Green
Kam Arnold
Blake D. Sherwin
Joaquin Vieira
Tijmen de Haan
Marilena LoVerde
M. Lilley
Marco Peloso
Raphael Flauger
John M Kovac
Josquin Errard
Scott Watson
Cora Dvorkin
Tristan L. Smith
Stephen M. Feeney
P. D. Meerburg
Sperello di Serego Alighieri
Akito Kusaka
J. Colin Hill
Glenn D. Starkman
Zeeshan Ahmed
W. L. Holzapfel
George M. Fuller
Julian B. Muñoz
Maude Le Jeune
Chao-Lin Kuo
Nathan Whitehorn
Adam Mantz
Reijo Keskitalo
Marcel Schmittfull
Christian L. Reichardt
Julian Borrill
Victor Buza
Michael D. Niemack
Emmanuel Schaan
Giulio Fabbian
Simone Ferraro
T. M. Crawford
Lorenzo Sorbo
Mathew S. Madhavacheril
Jeff McMahon
Ely D. Kovetz
Kevork N. Abazajian
James G. Bartlett
Jason W. Henning
Lloyd Knox
Evan Grohs
J. Peloton
K. T. Story
Robert R. Caldwell
Erminia Calabrese
Francesco De Bernardis
Wayne Hu
Steven W. Allen
Levon Pogosian
Sarah Shandera
David J. E. Marsh
Amber Miller
Joel Meyers
Arthur Kosowsky
John E. Carlstrom
Carlo Baccigalupi
Joanna Dunkley
Kevin M. Huffenberger
C. Pryke
Jeffrey P. Filippini
Alexander van Engelen
Francis-Yan Cyr-Racine
Bradford Benson
Marco Raveri
Daniel Grin
Colin A. Bischoff
Ho Nam Nguyen
Neelima Sehgal
Aditya Rotti
C. L. Chang
Vera Gluscevic
Douglas Scott
W. L. Kimmy Wu
David Alonso
Adrian T. Lee
Renée Hlozek
Graca Rocha
Peter Adshead
Gilbert Holder
Publication Year :
2016
Publisher :
Office of Scientific and Technical Information (OSTI), 2016.

Abstract

This book lays out the scientific goals to be addressed by the next-generation ground-based cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated telescopes at the South Pole, the high Chilean Atacama plateau and possibly a northern hemisphere site, all equipped with new superconducting cameras. CMB-S4 will dramatically advance cosmological studies by crossing critical thresholds in the search for the B-mode polarization signature of primordial gravitational waves, in the determination of the number and masses of the neutrinos, in the search for evidence of new light relics, in constraining the nature of dark energy, and in testing general relativity on large scales.

Details

Database :
OpenAIRE
Accession number :
edsair.doi...........0c3355cd5448743e76305fa52aa7ea5e
Full Text :
https://doi.org/10.2172/1352047